Data analysis for precision 21 cm cosmology
A Liu, JR Shaw - Publications of the Astronomical Society of the …, 2020 - iopscience.iop.org
The redshifted 21 cm line is an emerging tool in cosmology, in principle permitting three-
dimensional surveys of our universe that reach unprecedentedly large volumes, previously …
dimensional surveys of our universe that reach unprecedentedly large volumes, previously …
21 cm cosmology in the 21st century
Imaging the Universe during the first hundreds of millions of years remains one of the
exciting challenges facing modern cosmology. Observations of the redshifted 21 cm line of …
exciting challenges facing modern cosmology. Observations of the redshifted 21 cm line of …
Fundamental physics with the square kilometre array
The Square Kilometre Array (SKA) is a planned large radio interferometer designed to
operate over a wide range of frequencies, and with an order of magnitude greater sensitivity …
operate over a wide range of frequencies, and with an order of magnitude greater sensitivity …
Late-time cosmology with 21 cm intensity map** experiments
We present a framework for forecasting cosmological constraints from future neutral
hydrogen intensity map** experiments at low to intermediate redshifts. In the process, we …
hydrogen intensity map** experiments at low to intermediate redshifts. In the process, we …
64 constraints on reionization: the 21 cm power spectrum at z= 8.4
In this paper, we report new limits on 21 cm emission from cosmic reionization based on a
135 day observing campaign with a 64-element deployment of the Donald C. Backer …
135 day observing campaign with a 64-element deployment of the Donald C. Backer …
Science with the murchison widefield array
Significant new opportunities for astrophysics and cosmology have been identified at low
radio frequencies. The Murchison Widefield Array is the first telescope in the southern …
radio frequencies. The Murchison Widefield Array is the first telescope in the southern …
Measurement of 21 cm brightness fluctuations at z∼ 0.8 in cross-correlation
In this Letter, 21 cm intensity maps acquired at the Green Bank Telescope are cross-
correlated with large-scale structure traced by galaxies in the WiggleZ Dark Energy Survey …
correlated with large-scale structure traced by galaxies in the WiggleZ Dark Energy Survey …
A per-baseline, delay-spectrum technique for accessing the 21 cm cosmic reionization signature
ABSTRACT A critical challenge in measuring the power spectrum of 21 cm emission from
cosmic reionization is compensating for the frequency dependence of an interferometer's …
cosmic reionization is compensating for the frequency dependence of an interferometer's …
New limits on 21 cm epoch of reionization from paper-32 consistent with an x-ray heated intergalactic medium at z= 7.7
We present new constraints on the 21 cm Epoch of Reionization (EoR) power spectrum
derived from three months of observing with a 32 antenna, dual-polarization deployment of …
derived from three months of observing with a 32 antenna, dual-polarization deployment of …
H i constraints from the cross-correlation of eBOSS galaxies and Green Bank Telescope intensity maps
We present the joint analysis of Neutral Hydrogen (H i) Intensity Map** observations with
three galaxy samples: the Luminous Red Galaxy (LRG) and Emission Line Galaxy (ELG) …
three galaxy samples: the Luminous Red Galaxy (LRG) and Emission Line Galaxy (ELG) …